@InProceedings{MarranghelloAraś:2006:DeNeSt,
author = "Marranghello, Guilherme F. and Ara{\'u}jo, Jos{\'e} Carlos
Neves",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Determining the neutron star equation of state from gravitational
wave detections",
booktitle = "Anais...",
year = "2006",
organization = "Reuni{\~a}o Anual da Sociedade Astron{\^o}mica Brasileira, 32.",
abstract = "We briefly review the properties of quasi-normal modes of neutron
stars and black holes. Specially addressing our study to the
Brazilian spherical antenna, on which a possible detection would
occur at 3.0-3.4 kHz, we analyze the consequences of a possible
detection of such quasi-normal modes. Since the source can be
identified, by its characteristic damping time, we are able to
extract information about the neutron star or black hole. These
informations lead to a strong constraint in the nuclear matter
equation of state, namely, the compression modulus should be
K»220MeV.",
conference-location = "Atibaia, SP",
conference-year = "30 jul - 03 ago",
label = "self-archiving-INPE-MCTIC-GOV-BR",
language = "pt",
organisation = "Sociedade Astron{\^o}mica Brasileira",
targetfile = "marranghello_determining.pdf",
urlaccessdate = "02 maio 2024"
}